Table 4.
Statistics of the Gaussian approximating the RC stellar population within the investigated region.
| r | g0RCf | g0RC |
|---|---|---|
| 2.0°–2.1° | – | 19.5 ± 0.2 |
| 2.1°–2.2° | – | 19.5 ± 0.2 |
| 2.2°–2.3° | – | 19.5 ± 0.2 |
| 2.3°–2.5° | – | 19.5 ± 0.2 |
| 2.5°–2.6° | – | 19.5 ± 0.2 |
| 2.6°–2.8° | – | 19.5 ± 0.3 |
| 2.8°–3.1° | 19.3 ± 0.2 | 19.7 ± 0.1 |
| 3.1°–3.3° | 19.3 ± 0.2 | 19.7 ± 0.1 |
| 3.3°–3.6° | 19.3 ± 0.2 | 19.7 ± 0.1 |
| 3.6°–4.0° | 19.3 ± 0.2 | 19.7 ± 0.1 |
| 4.0°–4.6° | 19.2 ± 0.2 | 19.7 ± 0.1 |
| 4.6°–12.2° | 19.2 ± 0.2 | 19.6 ± 0.1 |
| 4.0°–4.1° | 19.2 ± 0.1 | 19.6 ± 0.2 |
| 4.1°–4.3° | 19.2 ± 0.2 | 19.7 ± 0.1 |
| 4.3°–4.6° | 19.3 ± 0.3 | 19.7 ± 0.0 |
| 4.6°–5.0° | 19.2 ± 0.2 | 19.7 ± 0.1 |
| 5.0°–5.6° | 19.1 ± 0.1 | 19.5 ± 0.2 |
| 5.6°–10.0° | – | 19.5 ± 0.3 |
Notes. The first column shows the inner and outer radii from the SMC centre of the analysed annulus. In the second and third columns, we inserted the mean and standard deviation of the Gaussians representative of the foreground population, if detected, and the main SMC population, respectively.
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